A survey for radio pulsars and transients in the 10 pc region around Sgr A*

Here we report on a new survey for pulsars and transients in the 10 pc region around Sgr A ∗ using the Effelsberg radio telescope at frequencies between 4 and 8 GHz. Our calibrated full-Stokes data were searched for pulsars and transients using PULSARX, TRANSIENTX, and PRESTO. Polarisation information is used in the scoring of the candidates. Our periodicity acceleration and jerk searches allowed us to maintain good sensitivity towards binary pulsars in ≳10-h orbits. In addition, we performed a dedicated search in linear polarisation for slow transients. While our searches yielded no new discovery beyond the redetection of the magnetar SGR J1745−2900, we report on a faint single pulse candidate in addition to several weak periodicity search candidates. After thoroughly assessing our survey’s sensitivity, we determined that it is still not sensitive to a population of millisecond pulsars. Next generation radio interferometers can overcome the limitations of traditional single-dish pulsar searches of the Galactic Centre.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2025-12-17
DOI
https://doi.org/10.1051/0004-6361/202556381
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
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article

A survey for radio pulsars and transients in the 10 pc region around Sgr A*

F. Abbate, R. S. Wharton, Yunpeng Men, M. Kramer et al.
Astronomy and Astrophysics
Pulsars and Gravitational Waves Research
article

A survey for radio pulsars and transients in the 10 pc region around Sgr A*

F. Abbate, R. S. Wharton, Yunpeng Men, M. Kramer, Pablo Torné, Ralph P. Eatough, R. Karuppusamy, L. Shao, K. Liu, G. Desvignes
article en

Abstract

Here we report on a new survey for pulsars and transients in the 10 pc region around Sgr A ∗ using the Effelsberg radio telescope at frequencies between 4 and 8 GHz. Our calibrated full-Stokes data were searched for pulsars and transients using PULSARX, TRANSIENTX, and PRESTO. Polarisation information is used in the scoring of the candidates. Our periodicity acceleration and jerk searches allowed us to maintain good sensitivity towards binary pulsars in ≳10-h orbits. In addition, we performed a dedicated search in linear polarisation for slow transients. While our searches yielded no new discovery beyond the redetection of the magnetar SGR J1745−2900, we report on a faint single pulse candidate in addition to several weak periodicity search candidates. After thoroughly assessing our survey’s sensitivity, we determined that it is still not sensitive to a population of millisecond pulsars. Next generation radio interferometers can overcome the limitations of traditional single-dish pulsar searches of the Galactic Centre.

Astronomy and AstrophysicsVol. 706
Chinese Academy of Sciences (CN), Shanghai Astronomical Observatory (CN), University of Manchester (GB), Instituto de Radioastronomía Milimétrica (ES), Osservatorio Astronomico di Cagliari (IT), Max Planck Institute for Radio Astronomy (DE), National Astronomical Observatories (CN)
Openalex Percentile: Top 72%
Pulsars and Gravitational Waves Research
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A survey for radio pulsars and transients in the 10 pc region around Sgr A* — F. Abbate, R. S. Wharton, et al. · Astronomy and Astrophysics (2025) | TGRS Research Map | TGRS